The final dataset we use is a set of uncorrelated data points from different  BAO measurements: the Sloan Digital Sky Survey (SDSS), the WiggleZ Dark Energy Survey, Dark Energy Camera Legacy Survey (DECaLS), the Dark Energy Survey (DES), the 6dF Galaxy Survey (6dFGS)
([1]}, [2]}, [3]}, [4]}, [5]}, [6]}, [7]}, [8]}, [9]}, [10]}, [11]}, [12]}, [13]}, [14]}, [15]}, [16]}). To this dataset, we add cosmic chronometers (CCs) (30 uncorrelated CC measurements of \(H(z)\)  [17]}, [18]}, [19]}, [20]}), and standard candles (SCs) (the Pantheon Type Ia supernova dataset [21]}, [22]}, [23]}, [24]}), and quasars [25]} and gamma-ray bursts [26]} (186 points).
